Emissivities for the various Graviton Modes in the Background of the Higher-Dimensional Black Hole
| dc.creator | Park, D. K. | |
| dc.date | 2006-03-29 | |
| dc.date | 2006-05-12 | |
| dc.date.accessioned | 2026-07-07T10:46:19Z | |
| dc.date.available | 2026-07-07T10:46:19Z | |
| dc.description | The Hawking emissivities for the scalar-, vector-, and tensor-mode bulk gravitons are computed in the full range of the graviton's energy by adopting the analytic continuation numerically when the spacetime background is $(4+n)$-dimensional non-rotating black hole. The total emissivity for the gravitons is only 5.16% of that for the spin-0 field when there is no extra dimension. However, this ratio factor increases rapidly when the extra dimensions exist. For example, this factor becomes 147.7%, 595.2% and 3496% when the number of extra dimensions is 1, 2 and 6, respectively. This fact indicates that the Hawking radiation for the graviton modes becomes more and more significant and dominant with increasing the number of extra dimensions. | |
| dc.description | 14 pages, 5 eps figures, V2: the incorrect multiplicities are corrected. PLB version | |
| dc.identifier | https://arxiv.org/abs/hep-th/0603224 | |
| dc.identifier | http://arxiv.org/abs/hep-th/0603224 | |
| dc.identifier | Phys.Lett.B638:246-252,2006 | |
| dc.identifier | doi:10.1016/j.physletb.2006.05.043 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/183191 | |
| dc.subject | High Energy Physics - Theory | |
| dc.title | Emissivities for the various Graviton Modes in the Background of the Higher-Dimensional Black Hole | |
| dc.type | text |